According to Britannica's article on Hipparchus, " ... observed the
positions of the stars and compared his results with those of Timocharis of
Alexandria about 150 years earlier and with even earlier observations made
in Babylonia....  He proposed precession to account for the size of the
difference and he gave a value of 45 or 46 (seconds of arc) for the annual
change, very close to the figure of 50.26 accepted today. ... Knowledge of
precession enabled him to obtain a better value for the length of the year
... his value for the tropical year was too great by only 6 1/2 [minutes?]".

So, indeed, he had access to a long series of observations, but it doesn't
answer the question of exactly how discovering precession led him to this
value.  Can anyone explain?

To note just two of his other achievements, he produced the first star
catalogue and was the first to specify position on the Earth by longitude
and latitude; surely, he was a very smart fellow indeed.


Andrew James

Reply via email to